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Coleman, in his notes, uses the statement "In NRQM, rotational invariance simplifies scattering problems." In general, I want to know how does it work? How does the rotational invariance help simplifying non-relativistic quantum scattering problems?

  1. One possibility is that if the Hamiltonian/potential is rotationally invariant, the scattering matrix is also rotationally invariant. But how does it simplify any scattering problem?

  2. What general conclusion can be drawn about the scattering amplitude for scattering from an arbitrary spherically symmetric potential?

It will be helpful if answers are supported by mathematical expressions/ or links.

SRS
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1 Answers1

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The simplification follows from the theorem which states that if such operator is conserved in Heisenberg sense, $$ \frac{d\hat{Q}}{dt} = \frac{\partial \hat{Q}}{\partial t} - \frac{i}{\hbar}[\hat{Q}, \hat{H}] = 0, $$ than it commutes with S-operator: $$ [\hat{Q}, \hat{S}] = 0 $$ So that these two operators can be diagonalized simulatenously: in corresponding basis $$ S_{\beta \alpha} = \langle \gamma{'}|\hat{S}|\gamma\rangle \delta_{\alpha \beta}, $$ where $\gamma$ is the full set of quantum numbers (charge, momentum etc) except the conserved integrals $\alpha, \beta$.

Suppose now we have the representation of S-matrix given by angles which define directions of incoming/outcoming particles, and there is rotational symmetry. We want to transform this representation to angular momentum representation. It can be done by using theorem stated above: $$ \langle \mathbf n{'}, \alpha|\hat{S}|\mathbf n, \beta \rangle = \sum_{l, l{'}}\sum_{m, m{'} = -l, l_{'}}^{l, l{'}}\langle \mathbf n{'}|l{'}, m{'}\rangle\langle l{'}, m{'}|\hat{S}_{\alpha \beta}|l, m\rangle \langle l, m|\mathbf n\rangle = $$ $$ \left| \langle l, m| \mathbf n\rangle = Y_{l,m}(\mathbf n), \quad \langle l{'}, m{'}|\hat{S}|l, m\rangle = \delta_{mm{'}}\delta_{ll{'}}S_{l}, \quad \sum_{m = -l}^{l}Y_{lm}(\mathbf n{'})Y_{lm}^{*}(\mathbf n) = \frac{2l+1}{4\pi}P_{l}(\cos (\theta )) \right| $$ $$ =\frac{1}{4\pi}\sum_{l}(2l+1)S^{l}_{\alpha \beta}P_{l}(\cos(\theta)), $$ where $\theta $ is an angle between $\mathbf n, \mathbf n{'}$. So that the scattering cross section is given by $$ \sigma_{\beta \to \alpha} = \frac{\pi}{k^{2}}\sum_{l = 0}^{\infty}(2l+1)\sum_{\beta \neq \alpha}|S^{l}_{\alpha \beta}|^{2} = \frac{\pi}{k^2}\sum_{l = 0}^{\infty}(2l+1)(1-|S_{\beta \beta}^{l}|^{2}) $$ So that you see that due to rotational symmetry cross section is completely determined by only only one diagonal S-matrix element $S^{l}_{\beta \beta}$. There is some additional information: if $|S_{\beta \beta}^{l}| = 1$ then the scattering cross-section $\beta \neq$ is zero. In such case scattering cross section with $\alpha \alpha$ is completely determined through so-called scattering phase $\delta_{l}$, $S_{\alpha \alpha}^{l} = e^{2i\delta_{l}}$.

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